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OSTP memo guides space nuclear plan
A White House Office of Science and Technology Policy (OSTP) memorandum released on Tuesday guides NASA, the Department of Energy, and the Department of Defense on their roles in deploying near-term space nuclear power.
This follows a series of NASA announcements last month—driven by the executive order “Ensuring American Space Superiority,” issued by Trump in December—including an ambitious timeline for establishing a moon base, which would rely on fission surface power (FSP) to survive the long lunar night at the moon’s south pole, and plans for a nuclear electric propulsion (NEP) rocket to be launched in 2028.
Imam Kambali, Angga Dwi Saputra, Marlina Marlina, Isdandy Rezki Febrianto, Ihwanul Aziz, Wira Y Rahman, Kristedjo Kurnianto, Rasito Tursinah, Rien Ritawidya, Ratna Dini Haryuni, Parwanto Parwanto, Rajiman Rajiman, Nur Huda, Kartika Fajarwati
Nuclear Science and Engineering | Volume 199 | Number 5 | May 2025 | Pages 829-837
Research Article | doi.org/10.1080/00295639.2024.2392070
Articles are hosted by Taylor and Francis Online.
The target holder, as part of the target system for cyclotron-based radioisotope production, plays a crucial role in successful radioisotope production. The target holder has to be designed and developed so that it will not deform or melt should a beam of energetic particles irradiate the target. In this work, we develop and test a target holder for 64Cu radioisotope production. The thermal distribution and structural analysis are simulated using ANSYS software. Based on the ANSYS simulation results, a maximum temperature of 84°C occurred on the titanium foil, while the maximum temperature in the target holder body was 35.6°C when an 11-MeV proton beam with a beam current of 25 μA was bombarded on the target holder.
We successfully test the target holder, and for the first time, we experimentally produce a 64Cu radioisotope by secondary neutron irradiation of the 64ZnO target. Using 11-MeV protons with a proton beam current of 25 μA incident on a 1-mm Ti foil for 5 min, we were able to generate secondary neutrons, and then the secondary neutrons irradiated 1 g of the enriched 64ZnO target. Copper-64 produced from the 64Zn(n,p)64Cu nuclear reaction was eventually detected using a portable gamma spectrometer, and its radioactivity was measured using a dose calibrator. For the first time, this experimental study confirmed that as much as 48.8 ± 6.2 MBq/μAh radioactivity of 64Cu was produced with no observed radioactive impurities.